Agenda and Program
Agenda and Program
The program was crafted by the science organizing committee, and only included invited talks:
Tuesday, August 19– General Reviews
8:00 – 8:30 Coffee
8:30 – 8:40 Welcome & Introduction
Charles Alcock, director (SAO)
Larry Ramsey, SOC chair (Penn State)
Session I. General review talks chair: Larry Ramsey
8:40 – 9:30 Overview: optical fibers in astronomy - today and tomorrow
Sam Barden (AIP) and Gabor Furesz (SAO)
9:30 – 10:30 Fiber manufacturing
Teodor Tichindelean (Polymicro)
10:30 – 10:45 Coffee
10:45 – 11:45 Theoretical studies and tools
Jeremy Allington-Smith (Durham Univ.)
11:45 – 12:45 Fiber termination/end processing, fiber characterization
Gabor Furesz (SAO)
Dionne Haynes (InnofSPEC)
12:45 – 14:00 Lunch
Session II. General review talks, cntd. chair: Sam Barden
14:00 – 15:00 Light injection and transport
Jon Lawrence (AAO)
15:00 – 16:00 Fiber positioners
Andy Sheinis (AAO)
16:00 – 16:20 Coffee
16:20 – 17:20 Lab visits (laser frequency comb, fiber characterization lab)
Wednesday, August 20 – Specific Applications & Techniques
8:00 – 8:30 Coffee
Session III. 3D/IFU spectroscopy (General review talks, finish) chair: Jon Lawrence
8:30 – 9:30 Thoughtful design and calibration of fiber fed instruments
Debra Fischer (Yale)
Francesco Pepe (Geneva Obs.)
9:30 – 10:15 IFU and IFU-based survey design: details from hardware
through software to science
Niv Drory (UT Austin)
Matt Bershady (Univ. of Wisconsin)
10:15 – 10:30 Coffee
10:30 – 11:30 IFUs from experience – CALIFA, SAMI and VENGA
Guillermo Blanc (Carnegie Obs.)
Julia Bryant (Univ. of Sidney)
Sebastian Sanchez (CAHA)
11:30 – 12:15 The VIRUS fiber system: design, fabrication, characterization
and data reduction issues
Gary Hill (UT Austin)
Andreas Kelz (AIP)
12:15 – 13:15 Lunch
13:15 – 14:00 IFUs for spectro-polarimetry applications
Haosheng Lin (Univ. of Hawaii)
Session IV. Speciality fibers chair: Gary Hill
14:00 – 14:45 Pioneering/developing of PCFs, multicore fibers and
photonic lanterns for astronomy specific development
Itandehui Gris Sanchez (Univ. of Bath)
14:45 – 15:30 Multicore fibers, fused fiber bundles and taper transitions
Dionne Haynes (InnofSPEC)
Sergio Leon-Saval (Univ. of Sidney)
15:30 – 15:45 Coffee
15:45 – 16:30 Fiber Bragg gratings and Photonics filters
Roger Haynes (InnofSPEC)
Simon Ellis (AAO)
16:30 – 17:15 Fiber based beam combiners, large mode area fibers,
few mode fibers
Joss Bland-Hawthorn (Univ. of Sidney) – remote talk
Thursday, August 21 – Specific Applications & Techniques, cntd.
8:00 – 8:30 Coffee
Session V. Planar and 3D waveguide structures chair: Roger Haynes
8:30 – 9:15 Pioneering the development of planar and 3D waveguide
structures in Astronomy
Robert Thomson (Heriot Watt Univ)
Nemanja Jovanovic (Subaru)
9:15 – 10:00 Integrated instrumentaion
Nick Cvetojevic (Univ. of Sidney)
10:15 – 10:30 Coffee
Session VI. High precision velocimetry and wavelength calibration chair: Debra Fischer
10:30 – 11:15 Fibers for PRV spectroscopy
Gerardo Avila (ESO)
11:15 – 12:00 Fibers in laser frequency combs
David Phillips (SAO)
12:00 – 13:00 Lunch
Session VII. Infrared fibers, interferometry, ELT instrumentation chair: Dionne Haynes
13:00 – 13:45 Mid-infrared fibers and photonics in astronomy
Suvrath Mahedavan (Penn State)
Lucas Labadie (Univ. of Köln)
13:45 – 14:30 GRAVITY - The VLT 4-beam combiner for narrow-angle astrometry and
interferometric imaging
Nicolas Blind (MPA)
14:30 – 15:15 Efficient single-mode fiber/photonic lantern injection with extreme adaptive
optics: enabling precision radial velocity and long baseline interferometry
Nemanja Jovanovic (Subaru)
15:15 – 15:30 Coffee
15:30 – 16:30 Fibers, fiber based instrumentations in the ELT era
Martin Roth (AIP)
John Pazder (Natnl. Research Council)
16:30 – 17:30 Open discussion, wrap-up
lead: Gabor Furesz
Some further details about the review talks:
Introductory talk:
Optical fibers in astronomy - today and tomorrow (60 min talk)
present/future landscape:
-science cases calling for/benefiting from using fibers (MOS, IFU, dIFU, interferometry), which are the major areas of interest today and tomorrow, what will be addressed during this workshop
brief historical review:
-overview of where we left off with Fiber Optics in Astronomy (FOiA) III, what were the major developments in the past 15 years
-major fiber instruments of the past 15 years, being built or planned
-who are the people and where are the active groups doing active fiber development
-review of resources
REVIEW talks:
35 - 45 min talks – allowing for up to 15 min discussion
R1: Fiber manufacturing
-manufacturing basics and techniques, what has changed, what precision of process control can be achieved, how does it affect quality, quality control
-materials: control of NA, what are the changes in materials, improvements, future promises
-preforms: capabilities, limitations, geometries,
-protective jacketing
-developments, costs, custom metrials, custom preforms, manufacturing constraints
-transmission, control over properties, etc.
(Polymicro, Ceramoptec, Fiberware, ??? etc.)
R2: Theoretical studies and tools
-theory of light propagation/FRD/scrambling
-modeling approaches (ray tracing, modal decomposition, beam propagation, etc.)
-computational methods, software tools
-modeling predictions vs. experimental results
-specialty fibers: PCFs, multicore, etc. – how to handle these in modeling (more on specialty fibers in a separate session)
R3: Fiber termination/end processing, fiber characterization
-cleaving and polishing: pros and cons, inspection, quality control, devices for processing and evaluation
-fiber processing: splicing, tapering, end caps, end polish; devices and evaluation techniques, quality control
-AR coatings: low-temp coatings, more complex coatings with splicing, evaluation
-characterization: throughput, FRD, modal structure, scrambling, near/far field; equipment to measure, repeatability, consistency of methods
-who does these, are there standards?
R4: Fiber connectors, fiber protection/packaging/handling
this talk was cancelled
-mounting fibers: temporary (testing) vs. permanent mounts, connector standards, stress, FRD consequences
-low-loss modular connectors, multiple fiber connectors: transmission, wear, repeatability, implications on FRD
-environmental protection, packaging (single, multiple, high multiplex), fiber bundle management
-dealing with thermal and mechanical stress, wear (fatigue over time), FRD implications
R5: “handling” light before/within/after a fiber link
-image feed and/vs. pupil feed: what does it mean for the instrument design/science
-use of micro/rod/GRIN lenses, beam homogenizers
-fiber end “sculpting” (more on these under 3D/IFU session and talk Highly multiplexed spectroscopy)
-numerical aperture, tapers, focal ratio conversion
-feeding calibration light (mimicking telescope feed to match stellar data)
-modal noise, modal scrambling
-scattered light (how to deal with the FRD losses)
R6: Multi-object and highly multiplexed spectroscopy
(more emphasis on positioners since more details in separate session on IFUs)
-plugplates, robots with plates and magnetic buttons, r-theta positioners, Echidna, hexabugs (2dF, 6dF, OzPoz/FLAMES, FMOS, WFMOS, DESI, 4MOST, also LAMOST, WEAVES, MOONS)
-high fill factor bundles (hexabundles, square tiles, IFUs) as part of MOS probe systems
-IFU design basics, differences/integration to MOS
R7: Thoughtful design and calibration of fiber fed instruments
-flat fielding, sky subtraction, photometric and spectrophotometric calibration
-what are the error sources and how could those be eliminated by design, calibration or special observing techniques
-what are the implication (or limitations imposed) on the science cases
-data simulation: generation of highly realistic artificial data to aid/advise instrument design, help developing data reduction tools
updated: 10/22/2014
updated: 10/22/2014
contact: gfuresz at mit . edu